Yoshimura Toshihiro, Takano Yoshinori, Naraoka Hiroshi, Koga Toshiki, Araoka Daisuke, Ogawa Nanako O, Schmitt-Kopplin Philippe, Hertkorn Norbert, Oba Yasuhiro, Dworkin Jason P, Aponte José C, Yoshikawa Takaaki, Tanaka Satoru, Ohkouchi Naohiko, Hashiguchi Minako, McLain Hannah, Parker Eric T, Sakai Saburo, Yamaguchi Mihoko, Suzuki Takahiro, Yokoyama Tetsuya, Yurimoto Hisayoshi, Nakamura Tomoki, Noguchi Takaaki, Okazaki Ryuji, Yabuta Hikaru, Sakamoto Kanako, Yada Toru, Nishimura Masahiro, Nakato Aiko, Miyazaki Akiko, Yogata Kasumi, Abe Masanao, Okada Tatsuaki, Usui Tomohiro, Yoshikawa Makoto, Saiki Takanao, Tanaka Satoshi, Terui Fuyuto, Nakazawa Satoru, Watanabe Sei-Ichiro, Tsuda Yuichi, Tachibana Shogo
Biogeochemistry Research Center (BGC), Japan Agency for Marine-Earth Science and Technology (JAMSTEC), Natsushima 2-15, Yokosuka, Kanagawa, 237-0061, Japan.
Department of Earth and Planetary Sciences, Kyushu University, 744 Motooka, Nishi-ku, Fukuoka, 819-0395, Japan.
Nat Commun. 2023 Sep 18;14(1):5284. doi: 10.1038/s41467-023-40871-0.
Samples from the carbonaceous asteroid (162173) Ryugu provide information on the chemical evolution of organic molecules in the early solar system. Here we show the element partitioning of the major component ions by sequential extractions of salts, carbonates, and phyllosilicate-bearing fractions to reveal primordial brine composition of the primitive asteroid. Sodium is the dominant electrolyte of the salt fraction extract. Anions and NH are more abundant in the salt fraction than in the carbonate and phyllosilicate fractions, with molar concentrations in the order SO> Cl> SO> NO> NH. The salt fraction extracts contain anionic soluble sulfur-bearing species such as S-polythionic acids (n < 6), C-alkylsulfonates, alkylthiosulfonates, hydroxyalkylsulfonates, and hydroxyalkylthiosulfonates (n < 7). The sulfur-bearing soluble compounds may have driven the molecular evolution of prebiotic organic material transforming simple organic molecules into hydrophilic, amphiphilic, and refractory S allotropes.
来自碳质小行星(162173)龙宫的样本提供了关于早期太阳系中有机分子化学演化的信息。在这里,我们通过对盐、碳酸盐和含页硅酸盐部分进行顺序萃取,展示了主要成分离子的元素分配情况,以揭示原始小行星的原始卤水成分。钠是盐部分提取物中的主要电解质。阴离子和NH在盐部分中比在碳酸盐和页硅酸盐部分中更丰富,摩尔浓度顺序为SO>Cl>SO>NO>NH。盐部分提取物包含阴离子可溶性含硫物种,如S-多硫代磺酸(n<6)、C-烷基磺酸盐、烷基硫代磺酸盐、羟烷基磺酸盐和羟烷基硫代磺酸盐(n<7)。这些含硫可溶性化合物可能推动了益生元有机物质的分子演化,将简单有机分子转化为亲水性、两亲性和难熔性的硫同素异形体。